Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data

dc.creatorWu, Puxun
dc.creatorYu, Hongwei
dc.date2006-12-09
dc.date.accessioned2026-07-07T11:21:35Z
dc.date.available2026-07-07T11:21:35Z
dc.descriptionWe examine observational constraints on the generalized Chaplygin gas (GCG) model for dark energy from the 9 Hubble parameter data points, the 115 SNLS Sne Ia data and the size of baryonic acoustic oscillation peak at redshift, $z=0.35$. At a 95.4% confidence level, a combination of three data sets gives $0.67\leq A_s\leq 0.83$ and $-0.21\leq α\leq 0.42$, which is within the allowed parameters ranges of the GCG as a candidate of the unified dark matter and dark energy. It is found that the standard Chaplygin gas model ($α=1$) is ruled out by these data at the 99.7% confidence level.
dc.description13 pages, 5 figures, to appear in PLB
dc.identifierhttps://arxiv.org/abs/gr-qc/0612055
dc.identifierhttp://arxiv.org/abs/gr-qc/0612055
dc.identifierPhys.Lett.B644:16-19,2007
dc.identifierdoi:10.1016/j.physletb.2006.11.028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194306
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGeneralized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
dc.typetext

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